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Galactic Chemical Evolution of the s Process from AGB Stars
A. Serminato, R. Gallino, C. Travaglio +2
We follow the chemical evolution of the Galaxy for the s elements using a Galactic chemical evolution (GCE) model, as already discussed by Travaglio et al. (1999, 2001, 2004), with…
Barium Stars: Theoretical Interpretation
L. Husti, R. Gallino, S. Bisterzo +2
Barium stars are extrinsic Asymptotic Giant Branch (AGB) stars. They present the s-enhancement characteristic for AGB and post-AGB stars, but are in an earlier evolutionary stage (…
Interpretation of CEMP(s) and CEMP(s + r) Stars with AGB Models
S. Bisterzo, R. Gallino, O. Straniero +1
Asymptotic Giant Branch (AGB) stars play a fundamental role in the s-process nucleosynthesis during their thermal pulsing phase. The theoretical predictions obtained by AGB models…
Properties of the 5- state at 839 keV in 176Lu and the s-process branching at A = 176
P. Mohr, S. Bisterzo, R. Gallino +3
The s-process branching at mass number A = 176 depends on the coupling between the high-K ground state and a low-lying low-K isomer in 176Lu. This coupling is based on electromagne…